Publication: Fermi Large Area Telescope Performance after 10 Years of Operation
dc.contributor.author | M. Ajello | en_US |
dc.contributor.author | W. B. Atwood | en_US |
dc.contributor.author | M. Axelsson | en_US |
dc.contributor.author | R. Bagagli | en_US |
dc.contributor.author | M. Bagni | en_US |
dc.contributor.author | L. Baldini | en_US |
dc.contributor.author | D. Bastieri | en_US |
dc.contributor.author | F. Bellardi | en_US |
dc.contributor.author | R. Bellazzini | en_US |
dc.contributor.author | E. Bissaldi | en_US |
dc.contributor.author | E. D. Bloom | en_US |
dc.contributor.author | R. Bonino | en_US |
dc.contributor.author | J. Bregeon | en_US |
dc.contributor.author | A. Brez | en_US |
dc.contributor.author | P. Bruel | en_US |
dc.contributor.author | R. Buehler | en_US |
dc.contributor.author | S. Buson | en_US |
dc.contributor.author | R. A. Cameron | en_US |
dc.contributor.author | P. A. Caraveo | en_US |
dc.contributor.author | E. Cavazzuti | en_US |
dc.contributor.author | M. Ceccanti | en_US |
dc.contributor.author | S. Chen | en_US |
dc.contributor.author | C. C. Cheung | en_US |
dc.contributor.author | S. Ciprini | en_US |
dc.contributor.author | I. Cognard | en_US |
dc.contributor.author | J. Cohen-Tanugi | en_US |
dc.contributor.author | S. Cutini | en_US |
dc.contributor.author | F. D'Ammando | en_US |
dc.contributor.author | P. De La Torre Luque | en_US |
dc.contributor.author | F. De Palma | en_US |
dc.contributor.author | S. W. Digel | en_US |
dc.contributor.author | F. Dirirsa | en_US |
dc.contributor.author | N. Di Lalla | en_US |
dc.contributor.author | L. Di Venere | en_US |
dc.contributor.author | A. Domínguez | en_US |
dc.contributor.author | D. Fabiani | en_US |
dc.contributor.author | E. C. Ferrara | en_US |
dc.contributor.author | A. Fiori | en_US |
dc.contributor.author | G. Foglia | en_US |
dc.contributor.author | Y. Fukazawa | en_US |
dc.contributor.author | P. Fusco | en_US |
dc.contributor.author | F. Gargano | en_US |
dc.contributor.author | D. Gasparrini | en_US |
dc.contributor.author | M. Giroletti | en_US |
dc.contributor.author | T. Glanzman | en_US |
dc.contributor.author | D. Green | en_US |
dc.contributor.author | S. Griffin | en_US |
dc.contributor.author | M. H. Grondin | en_US |
dc.contributor.author | J. E. Grove | en_US |
dc.contributor.author | L. Guillemot | en_US |
dc.contributor.author | S. Guiriec | en_US |
dc.contributor.author | M. Gustafsson | en_US |
dc.contributor.author | E. Hays | en_US |
dc.contributor.author | D. Horan | en_US |
dc.contributor.author | G. Jóhannesson | en_US |
dc.contributor.author | T. J. Johnson | en_US |
dc.contributor.author | T. Kamae | en_US |
dc.contributor.author | M. Kerr | en_US |
dc.contributor.author | M. Kuss | en_US |
dc.contributor.author | S. Larsson | en_US |
dc.contributor.author | L. Latronico | en_US |
dc.contributor.author | M. Lemoine-Goumard | en_US |
dc.contributor.author | J. Li | en_US |
dc.contributor.author | I. Liodakis | en_US |
dc.contributor.author | F. Longo | en_US |
dc.contributor.author | F. Loparco | en_US |
dc.contributor.author | M. N. Lovellette | en_US |
dc.contributor.author | P. Lubrano | en_US |
dc.contributor.author | S. Maldera | en_US |
dc.contributor.author | A. Manfreda | en_US |
dc.contributor.author | G. Martí-Devesa | en_US |
dc.contributor.author | M. N. Mazziotta | en_US |
dc.contributor.author | N. Menon | en_US |
dc.contributor.author | I. Mereu | en_US |
dc.contributor.author | M. Meyer | en_US |
dc.contributor.author | P. F. Michelson | en_US |
dc.contributor.author | M. Minuti | en_US |
dc.contributor.author | W. Mitthumsiri | en_US |
dc.contributor.author | T. Mizuno | en_US |
dc.contributor.author | M. Mongelli | en_US |
dc.contributor.author | M. E. Monzani | en_US |
dc.contributor.author | I. V. Moskalenko | en_US |
dc.contributor.author | M. Negro | en_US |
dc.contributor.author | E. Nuss | en_US |
dc.contributor.author | R. Ojha | en_US |
dc.contributor.author | M. Orienti | en_US |
dc.contributor.author | E. Orlando | en_US |
dc.contributor.author | A. Paccagnella | en_US |
dc.contributor.author | V. S. Paliya | en_US |
dc.contributor.author | D. Paneque | en_US |
dc.contributor.author | Z. Pei | en_US |
dc.contributor.author | J. S. Perkins | en_US |
dc.contributor.author | M. Pesce-Rollins | en_US |
dc.contributor.author | M. Pinchera | en_US |
dc.contributor.author | F. Piron | en_US |
dc.contributor.author | H. Poon | en_US |
dc.contributor.author | T. A. Porter | en_US |
dc.contributor.author | R. Primavera | en_US |
dc.contributor.author | G. Principe | en_US |
dc.contributor.author | J. L. Racusin | en_US |
dc.contributor.other | Oskar Klein Centre | en_US |
dc.contributor.other | Istituto Nazionale di Fisica Nucleare, Sezione di Trieste | en_US |
dc.contributor.other | Istituto Nazionale di Fisica Nucleare, Sezione di Perugia | en_US |
dc.contributor.other | Istituto Nazionale di Fisica Nucleare, Sezione di Lecce | en_US |
dc.contributor.other | Istituto Nazionale di Fisica Nucleare, Sezione di Bari | en_US |
dc.contributor.other | Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergata | en_US |
dc.contributor.other | Istituto Nazionale di Fisica Nucleare, Sezione di Torino | en_US |
dc.contributor.other | Istituto Nazionale di Fisica Nucleare, Sezione di Pisa | en_US |
dc.contributor.other | Istituto Nazionale Di Fisica Nucleare, Sezione di Padova | en_US |
dc.contributor.other | Laboratoire Univers et Particules de Montpellier | en_US |
dc.contributor.other | Santa Cruz Institute for Particle Physics | en_US |
dc.contributor.other | INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan | en_US |
dc.contributor.other | Raunvísindastofnun Háskólans | en_US |
dc.contributor.other | Laboratoire de Physique des 2 infinis de Bordeaux | en_US |
dc.contributor.other | Agenzia Spaziale Italiana | en_US |
dc.contributor.other | Georg-August-Universität Göttingen | en_US |
dc.contributor.other | Hiroshima University | en_US |
dc.contributor.other | Deutsches Elektronen-Synchrotron (DESY) | en_US |
dc.contributor.other | Universite d'Orleans | en_US |
dc.contributor.other | Università di Pisa | en_US |
dc.contributor.other | Stockholms universitet | en_US |
dc.contributor.other | Politecnico di Bari | en_US |
dc.contributor.other | Universidad Complutense de Madrid | en_US |
dc.contributor.other | Naval Research Laboratory | en_US |
dc.contributor.other | Clemson University | en_US |
dc.contributor.other | Laboratoire de Physique Subatomique et de Cosmologie de Grenoble | en_US |
dc.contributor.other | SLAC National Accelerator Laboratory | en_US |
dc.contributor.other | The University of Tokyo | en_US |
dc.contributor.other | University of Maryland, Baltimore County (UMBC) | en_US |
dc.contributor.other | Universita del Salento | en_US |
dc.contributor.other | University of Maryland, College Park | en_US |
dc.contributor.other | Université Savoie Mont Blanc | en_US |
dc.contributor.other | INSU - Institut National des Sciences de l'Univers | en_US |
dc.contributor.other | Università degli Studi di Trieste | en_US |
dc.contributor.other | George Mason University | en_US |
dc.contributor.other | Högskolan Dalarna | en_US |
dc.contributor.other | École polytechnique | en_US |
dc.contributor.other | Mahidol University | en_US |
dc.contributor.other | Julius-Maximilians-Universität Würzburg | en_US |
dc.contributor.other | Istituto Di Radioastronomia, Bologna | en_US |
dc.contributor.other | Università degli Studi di Torino | en_US |
dc.contributor.other | Universität Innsbruck | en_US |
dc.contributor.other | Max Planck Institute for Physics (Werner Heisenberg Institute) | en_US |
dc.contributor.other | Turun yliopisto | en_US |
dc.contributor.other | NASA Goddard Space Flight Center | en_US |
dc.contributor.other | The George Washington University | en_US |
dc.contributor.other | Università degli Studi di Perugia | en_US |
dc.contributor.other | The Royal Institute of Technology (KTH) | en_US |
dc.contributor.other | Friedrich-Alexander-Universität Erlangen-Nürnberg | en_US |
dc.contributor.other | Università degli Studi di Padova | en_US |
dc.date.accessioned | 2022-08-04T08:31:59Z | |
dc.date.available | 2022-08-04T08:31:59Z | |
dc.date.issued | 2021-09-01 | en_US |
dc.description.abstract | The Large Area Telescope (LAT), the primary instrument for the Fermi Gamma-ray Space Telescope (Fermi) mission, is an imaging, wide field-of-view, high-energy gamma-ray telescope, covering the energy range from 30 MeV to more than 300 GeV. We describe the performance of the instrument at the 10 yr milestone. LAT performance remains well within the specifications defined during the planning phase, validating the design choices and supporting the compelling case to extend the duration of the Fermi mission. The details provided here will be useful when designing the next generation of high-energy gamma-ray observatories. | en_US |
dc.identifier.citation | Astrophysical Journal, Supplement Series. Vol.256, No.1 (2021) | en_US |
dc.identifier.doi | 10.3847/1538-4365/ac0ceb | en_US |
dc.identifier.issn | 00670049 | en_US |
dc.identifier.other | 2-s2.0-85115774062 | en_US |
dc.identifier.uri | https://repository.li.mahidol.ac.th/handle/20.500.14594/76851 | |
dc.rights | Mahidol University | en_US |
dc.rights.holder | SCOPUS | en_US |
dc.source.uri | https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85115774062&origin=inward | en_US |
dc.subject | Earth and Planetary Sciences | en_US |
dc.subject | Physics and Astronomy | en_US |
dc.title | Fermi Large Area Telescope Performance after 10 Years of Operation | en_US |
dc.type | Article | en_US |
dspace.entity.type | Publication | |
mu.datasource.scopus | https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85115774062&origin=inward | en_US |